Pulsar Timing Arrays Current and Future Instrumentation - DCC

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$Numerical simulation of diffraction grating alignment and ... - DCC$

Pulsar Timing ArraysDigital BackendsWide-bandwidth (1+ GHz),real-time systemsimplementing RFImitigation and folding(in construction)• Parkes HIPSR• Effelsberg ASTERIX andfollow-on• Arecibo PUPPIClone of GBT GUPPIFPGA-based Reconfigurable Open Architecture ComputingHardware (ROACH), developed by Center for AstronomicalSignal Processing and Electronics Research (CASPER, at UCBerkeley)
Pulsar Timing ArraysNew Feed & Rx Systems• GBT Wide-Band PulsarSystem• Arecibo Wide-Band System• Effelsberg Ultra-broad Band• Arecibo AO40• Five-hundred metreAperture SphericalTelescope (FAST) multi-feedsystem19 or 100 feed hornsT sys ~ 29K (5K sky + 9K spill + 4K coax jct + 7K dewar jct + 3K LNA)
Page 1 and 2: Pulsar Timing ArraysCurrent and Fut
Page 3 and 4: Pulsar Timing ArraysCurrent Results
Page 5 and 6: Radio Telescope
Page 7 and 8: Radio TelescopeTNoise Temperature
Page 9 and 10: Pulsar ObservationsObservational fr
Page 11 and 12: Pulsar Timing ArraysCurrent Instrum
Page 13 and 14: Pulsar Timing ArraysCurrent Instrum
Page 15 and 16: Pulsar Surveysa “position” on t
Page 17: Green Bank Ultimate PulsarProcessin
Page 23 and 24: Pulsar Timing ArraysNew ApproachesS
Page 25 and 26: Pulsar Timing ArraysNew ApproachesF
Page 27 and 28: Pulsar Timing ArraysFuture Telescop
Page 29 and 30: Radio Telescopes andAstrophysical S

Pulsar Timing Arrays Current and Future Instrumentation - DCC

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